Monitoring of the optical and 2.5-11.7 mu m spectrum and mid-IR imaging of the Seyfert 1 galaxy Mrk 279 with ISO
Citations
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Cites background from "Monitoring of the optical and 2.5-1..."
...…suggested that the absence or suppression of UIB emission is due to the fact that the dust is predominantly heated by processes related to the central AGN [e.g. in NGC 1068 (Le Floc’h et al., 2001), Circinus (Moorwood, 1999), NGC 4151 (Sturm et al., 1999), Mrk 279 (Santos-Lleó et al., 2001)]....
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...…ISO monitoring of variable AGN, that were contemporaneous to other multiwavelength campaigns, failed to show any convincing thermal variability (e.g. Mrk 279 Santos-Lleó et al., 2001; BL Lac PKS 2155-304 Bertone et al., 2000; BL Lac 2007+777 Peng et al., 2000; OVV quasar 3C 446 Leech et al., 2002)....
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...In intense radiation fields ( 105 times that of the local ISRF) such as in metal poor environments or in the vicinity of super star clusters or AGN, UIBs are weak or absent (Contursi et al., 2000, Thuan et al., 1999, Rigopoulou et al., 1999, Sturm et al., 2000, Santos-Lleó et al., 2001)....
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55 citations
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Additional excerpts
...…et al. 1997; (4) Rodriguez-Pascual et al. 1997;(5) Stirpe et al. 1994; (6) Peterson et al. 2000; (7) Kaspi et al. 1996; (8) Crenshaw et al. 1996; (9) Santos-Lleo et al. 2001; (10) Wanders & Peterson 1996; (11) the UltraViolet Light Curve Database for AGNs; (12) Dietrich et al. 1998; (13) Carone et…...
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46 citations
References
1,139 citations
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"Monitoring of the optical and 2.5-1..." refers methods in this paper
...Reverberation-mapping techniques (Blandford & McKee 1982) have been used extensively to map the BLR in several AGN, on scales of light days to light months, notably by the International AGN Watch1 consortium (Alloin et al. 1994)....
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818 citations
"Monitoring of the optical and 2.5-1..." refers methods in this paper
...We used both the interpolation method of Gaskell & Sparke (1986) and the discretecorrelation function (DCF) method of Edelson & Krolik (1988), in both cases employing the specific implementation described by White & Peterson (1994)....
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648 citations
"Monitoring of the optical and 2.5-1..." refers background in this paper
...The presence of a universal inflection point near 1.2µm in the spectral energy distribution of radio-quiet AGN’s strongly suggests that the bulk of the near IR flux arises from dust thermal emission (e.g., Barvainis 1987; Sanders et al. 1989)....
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644 citations
"Monitoring of the optical and 2.5-1..." refers background in this paper
...The presence of a universal inflection point near 1.2µm in the spectral energy distribution of radio-quiet AGN’s strongly suggests that the bulk of the near IR flux arises from dust thermal emission (e.g., Barvainis 1987; Sanders et al. 1989)....
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